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| Paper IPM / P / 6733 |
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| Abstract: | |||||||||
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The dispersion relation for a dusty plasma containing elongated
and rotating charged dust grains is obtained by assuming that the
dipole moments of the dust particulates are nonzero. The
longitudinal waves with frequency close to the angular rotation
frequency of the dust grains are found to be unstable. The results
should be relevant to enhanced fluctuations in astrophysical
environments.
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